Submillimeter Spectroscopy of Low Temperature Gases

Details Submillimeter Spectroscopy of Low Temperature Gases Submillimeter Spectroscopy of Low Temperature Gases

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002dps....34.3903w&link_type=abstract

American Astronomical Society, DPS Meeting #34, #39.03; Bulletin of the American Astronomical Society, Vol. 34, p.910

Astronomy and Astrophysics

Astronomy

Scientific paper

Submillimeter absorption spectra of nitrogen, nitrogen-argon mixtures, methane, and CO-hydrogen mixtures have been measured at pressures and temperatures near to those found in the atmospheres of Titan and Saturn. The experiments show the spectra signatures of dimers which will likely appear in the far-infrared spectra of Titan and Saturn that will be obtained by the Composite Infrared Spectrometer (CIRS) onboard the Cassini spacecraft. The recent CIRS spectrum of Jupiter shows spectra lines of methane and the corresponding lines have been observed in the laboratory. New experimental data obtained with a differential Michelson interferometer and cryogenic abosorption cell system that operates over the frequency region 3--25 cm(-1) will be presented.

Affiliated with

Also associated with

No associations

Rating

Submillimeter Spectroscopy of Low Temperature Gases does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Submillimeter Spectroscopy of Low Temperature Gases, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Submillimeter Spectroscopy of Low Temperature Gases will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1045775